Holographic Cosmology 3.0*
Abstract
We present a new version of holographic cosmology, which is compatible with present observations. A primordial p = ρ phase of the universe is followed by a brief matter dominated era and a brief period of inflation, whose termination heats the universe. The flatness and horizon problems are solved by the p = ρ dynamics. The model is characterized by two parameters, which should be calculated in a more fundamental approach to the theory. For a large range in the phenomenologically allowed parameter space, the observed fluctuations in the cosmic microwave background were generated during the p = ρ era, and are exactly scale invariant. The scale invariant spectrum cuts off sharply at both upper and lower ends, and this may have observational consequences. We argue that the amplitude of fluctuations is small but cannot yet calculate it precisely.
 Publication:

Physica Scripta Volume T
 Pub Date:
 January 2005
 DOI:
 10.1238/Physica.Topical.117a00056
 arXiv:
 arXiv:hepth/0405200
 Bibcode:
 2005PhST..116...56B
 Keywords:

 High Energy Physics  Theory;
 Astrophysics;
 General Relativity and Quantum Cosmology;
 High Energy Physics  Phenomenology
 EPrint:
 This is an expanded version of an essay submitted to the Gravity Foundation Competition, 11 pages